Mission
2004: The Search for Life On Mars
by Cassie Rodriquez
Is there life on Mars? How would you begin to answer this question?
In the Fall of 2000, Mission 2004: The Search for Life On Mars was a new class
offered to freshman as part of an Institute-wide initiative to expand the horizons
of MIT undergraduate education. While most first year subjects deal with the
typical “problem set” and lecture type atmosphere, Mission 2004, taught by Professor
Kip Hodges, provided a unique opportunity to experience cross-disciplinary problem
solving in a collaborative learning environment. The students were assigned
the following task: Develop a viable mission plan for the exploration of Mars
with the aim of finding evidence for the present or past existence of life.
In teams, the students tackled various technical, scientific, and political
issues that would affect a Mars mission. Several questions were extensively
discussed and debated. For example, how do we define life? We decided on five
criteria for life, based on the energy properties of living systems rather the
than chemical properties.
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The landing site: Diacria Crater
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The following five basic charactertics were used as the definition of life
for this mission design: (1) shows evidence of growth and replication; (2) shows
evidence of purposeful energy transfer; (3) responds to stimuli; (4) acts in
such a way as to ensure self-preservation; and (5) is significantly different
from the surrounding environment.
After the definition of life was established and it was decided that the mission
should be manned, the details of the mission architecture began to fall into
place. But still numerous questions remained - how will the public react and
how much would they be willing to pay for a mission in search of life on Mars?
The Mission 2004 team looked into public relations through advertising and public
funding. A mission budget based on the percentage that NASA gave to the Apollo
program in the 1960’s and other Mars missions was estimated to be $140 billion
over 20 years.
How do we get to Mars? The extensive mission payload required advanced propulsion
systems to be adopted, separating experimental equipment and the human crew.
Surface transportation (rovers) were developed to handle the experimental packages.
Incorporated into all structures were life support methods and communication
systems. Life detecting methods included geological surveys, spectroscopic analysis,
organic analysis, and biological experiments. A timeline for the mission, which
included a breakdown of research, manufacturing, launch windows, travel/stay
time, was developed. This comprehensive plan embodies the semester of work entitled
Mission 2004: The Search for Life on Mars. The plan was presented formally to
the MIT community and two leading NASA scientists - Dr. Jack Farmer and Dr.
Jim Garvin. The Mission 2004 presentation and multi-media website, containing
further information, can be viewed at: http://web.mit.edu/12.000/www/home.html.
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The Mars Rover with trailers
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